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Paper Citation Record · LEDGER

The cometary HII regions of DR 21: Bow shocks or champagne flows or both?

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1401.1343.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1401.1343 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:56.985487Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: cited_works

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation e520eb10-3228-4d86-88d0-9a64b12f5d97 · inbound

Bipolar HII regions Produced by Cloud-Cloud Collisions cites this paper.

Bipolar HII regions Produced by Cloud-Cloud Collisions The cometary HII regions of DR 21: Bow shocks or champagne flows or both?

Reference 55

Resolution
unresolved
no resolver link, observed 2026-07-31T15:39:29.230709Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T15:39:29.230709Z digest=sha256:4bcfddde7e4b967b0549b451c0a9777e5ce8a39a1235b428661294580ad231a9

Observation dc91a6de-a30b-4964-8851-ccc88fd001c7 · inbound

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry The cometary HII regions of DR 21: Bow shocks or champagne flows or both?

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-07T20:40:56.985487Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T20:40:56.985487Z digest=sha256:fe35ed007ec2164f25a2acb9c728379afcd5831341abe20a0a12764a67acbd2f